Fluid-Maxwell simulation of laser pulse dynamics in overdense plasma

被引:24
作者
Berezhiani, VI [1 ]
Garuchava, DP
Mikeladze, SV
Sigua, KI
Tsintsadze, NL
Mahajan, SM
Kishimoto, Y
Nishikawa, K
机构
[1] Georgian Acad Sci, Inst Phys, GE-380077 Tbilisi, Georgia
[2] Univ Texas, Inst Fus Studies, Austin, TX 78712 USA
[3] JAERI, Naka Fus Res Estab, Naka, Ibaraki, Japan
[4] Kinki Univ, Fac Engn, Higashihiroshima, Japan
关键词
D O I
10.1063/1.1924708
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
A one-dimensional model of collisionless electron plasma, described by the full system of Maxwell and relativistic hydrodynamic equations, is exploited to study the interaction of relativistic, strong, circularly polarized laser pulses with an overdense plasma. Numerical simulations for the ultrarelativistic pulses demonstrates that for the low as well as for the high background density, the major part of the penetrated energy remains trapped for a long time in a nonstationary layer near the plasma front end; only a minor portion resides in solitons. Important details of the interaction for the moderately intense and strongly relativistic pulses for semi-infinite and thin plasma layers are revealed. An interesting additional consequence of the long-time confinement of relativistic strong radiation in an overdense plasma is analyzed. It is shown that intensive pair production by the driven motion of plasma electrons takes place due to the trident process. (C) 2005 American Institute of Physics.
引用
收藏
页码:1 / 14
页数:14
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